Now widely accepted as the construction industry's standard measure of safety performance, the STEP awards were established in 1989 to evaluate and improve safety practices and recognize outstanding safety efforts.

A recent study by Mingus Union High School administration showed Cottonwood Middle School students passed the science portion of the Arizona's Instrument to Measure Standards test at a much higher rate than MUHS students.

In science:

If Φ is a perturbed simply attractive model, then λ is easily seen to be a ﬁnite measure; we can add ∞ to E to make it a compact standard Borel space (by the deﬁnition of ) with ﬁnite underlying measure.

Random Surfaces

As can be seen from Figure 2 of Fontaine et al. (2003), the standard deviations between both sets of measurements allow us to estimate the real external errors for stars in the ZZ Ceti range, σ(Teff ) ∼ 200 K and σ(log g ) ∼ 0.05.

On the Purity of the ZZ Ceti Instability Strip: Discovery of More Pulsating DA White Dwarfs on the Basis of Optical Spectroscopy

We refer the reader to for standard results concerning the space of measures.

It is the second type of measurement which is considered here, which yields insight into single particle properties which differ from the standard ensemble measurement, provided that a non-ergodic phase is investigated.

A Random Walk to a Non-Ergodic Equilibrium Concept

First, it may be tempting to deﬁne a random element of a borelogical space V as a measurable map from a standard probability space Ω to the (nonstandard) measurable space (V, Σ).

Note that for every u and v in D, if the geodesic segment [u, v ] is transverse to Lg, then ed(u, v ) = dg (π(u), π(v )), as any piecewise transverse path from u to v has transverse measure at least the transverse measure of [u, v ], by standard arguments.

Scaling limits of bipartite planar maps are homeomorphic to the 2-sphere

We measured the probability of |1i as a function of time for the standard refocused decoherence measurement.

Randomized Benchmarking of Quantum Gates

A standard method of measuring rotational periods is based on observations of stellar surface inhomogeneities which produce signal modulations over the rotational period.

Then Ξn converges in distribution (with respect to the topology of weak convergence of probability measures on R) to a random probability measure Ξ∞ that is Gaussian with random mean θZ and nonrandom variance 1 − θ2, where Z is a standard Gaussian random variable.

Spectra of random linear combinations of matrices defined via representations and Coxeter generators of the symmetric group

In fact, for any real x and any measure µ one can ﬁnd a Cauchy sequence of measures in D such that a standard binary encoding ρµ of this sequence computes x, hence x is not random for µ with respect to the representation ρµ .

Measures and their random reals

Measurement of the coherent scattering cross-section would provide a sensitive test to the Standard Model11,12 probing the weak nuclear charge and radiative corrections due to possible non-standard neutrino interactions or additional neutral gauge bosons.